Showing posts with label Jovian Dual Transit. Show all posts
Showing posts with label Jovian Dual Transit. Show all posts

Wednesday, February 29, 2012

The Rare Triple Eclipse of Jupiter

Written by Matthew Winter 

On March 28, 2004, The Hubble Space Telescope snapped an amazing picture of the transit of two of Jupiter’s confirmed sixty-six moons, and the shadows of three of them, resulting in an image of which shows the spontaneous phenomena capable of this planet’s lunar bodies. At first glances, Jupiter appears to be a brightly colored orb, with hues parallel to a pastel or neon painting, with five different spots placed randomly about its northern hemisphere; its altered coloring was result of being taken by Hubble’s Near Infrared Camera and Multi-Object Spectrometer, instead of photographing in the visible spectrum. The image is comprised of three of these near-infrared photographs, producing the different shades of color visible—yellow indicates high cloud cover, red indicates low, and blue, even lower cloud cover. 


 Although phenomena such as the event captured in the image, finding Jupiter in the night sky is no hard task and can be especially bight when at opposition. But, there are no definite set of celestial coordinates in locating this planet, because of its ever-changing position in the night sky. According to ephemerides however, computers have been able to plot the course of Jupiter on timescales greater than one millennium, so locating and charting the planet’s position will never be tedious work. For the end of February 2012, Jupiter will be visible in the south-southwestern sky just after sunset, at the averaged Right Ascension of 2h 19m and the Declination of + 12° 53’. Again, phenomena seen in the image are rare and do not occur often.

Upon looking at the image, you might inquire of when such an event will occur on Jupiter. Although it might seem very rare that three moons cast their shadow while two transit, rather it is not. This event is called a Jovian Dual-Transit, as it incorporates two different moons, in this case Io and Ganymede, simultaneously transit the surface. But because of the two shadows also cast by these two moons, it is more appropriately named A Jovian Dual-Shadow Transit where two moons transit and cast shadows. The third shadow, consequently given by Callisto, not pictured in the image, makes this event even more complex—and it is quite spectacular that Hubble was in the right place at the right time to photograph such a spectacle. In describing it, however, it is not troublesome to locate the three, distinct shadows of the three moons notwithstanding Io and Ganymede, which seem to be camouflaged in with Jupiter’s pallid colors. Io sits nearly in the center of the image, in white, opposed to its visible color of hazy yellow or golden. Ganymede is to the upper right of Io, and is pale blue; Ganymede is visibly the color of our Moon, a flushed grey.

Whereas a beautiful image of Jupiter with three shadows and two moons cresting its upper hemisphere is rather somber and dreamy, to astronomers, this image allowed them to attempt a new technique of imaging, which succeeded in the end. Attempting to capture images of Jupiter and its moon is rather difficult, especially when completely focused on an object. Because Jupiter moves quickly across Hubble’s telescope view, it was necessary to take a rapid succession of images, before Jupiter moved out of the telescope’s lenses.

Of course, Hubble has the equipment to track an object far away and hold for hours; Jupiter is much closer to earth than distant galaxies, so things tend to move quicker than you would think—and when locked onto it, the sharpness of the image was distorted, creating a blurry picture, not fit to be called a Hubble image. So, astronomers tried, for the purpose of creating a sharper, neater image, to speed up Hubble’s tracking system, resulting in the ‘slower’ movement of Jupiter through the telescope, which in return allowed Hubble to take such a fine image of its moon in such phenomena.

In conclusion, it is important to see that not only did this image of Jupiter’s rare triple ‘eclipse’ phenomena helped astronomers for the better of planetary images (in that, the slowing down of Hubble’s tracking system made clearer photographs of planets from earth), but also to record a rare event for the wonder and mystery of extraplanetary phenomena—other planets do indeed experience eclipses and transits!

With Information from (Accessed February 24 & 27 2012):

Sunday, January 22, 2012

Understanding Jovian Eclipses

[This article concerns Jovian eclipses, not transits. Although a Jovian eclipse can mean the same thing as a transit in this sense, this article talks about the disappearance and reappearance of the Jovian moons, not the transit of Jupiter’s surface.]

Considered the most intriguing and fascinating astronomical phenomena yet, the eclipse is highly acclaimed not just here on earth, but also in the rest of our solar-system. When a celestial body passes into the shadow of another body, preferably larger; or an object casts a shadow upon another, an eclipse is formed. From there, the term ‘eclipse’ can be forwarded into two separate definitions: the solar eclipse, or the lunar eclipse. When the Moon passes in front of the Sun, respectively on the ecliptic, a shadow is cast upon the earth; a solar eclipse is formed. When the Moon passes into either the umbral or penumbral shadow of the earth, again respectively on the ecliptic; a lunar eclipse occurs. Although these definitions discreetly define actions in a terrestrial sense, these same exact phenomena occur on the other seven planets in our vast solar-system, but with another name.

When an object passes into the shadow cone of Jupiter, it disappears from view (note the striped moon to represent being eclipsed instead of being solid colored, not eclipsed)
The Jovian Eclipse is perhaps one of the most unique extraterrestrial happenings, for it involves one of the many Jovian moons, mainly the Galilean moons, Jupiter, and the Sun; rather just the Moon and earth. Because a solar eclipse and a lunar eclipse have terrestrial definitions and terms, therefore, a Jovian Eclipse is defined as “the passing of a Jovian moon into the shadow-cone of Jupiter where it is eclipsed out of sight, until reappearing.” These eclipses can be total, in which the eclipsed moon is eclipsed indefinitely; or partial, where the eclipsed moon is partially eclipsed. But, you must make note that the Galilean moons (the four most famous moons, which we do know to eclipse) have very little orbital inclinations. With Io, having an inclination of 0.050º, Europa with 0.471º, Ganymede with 0.204º, and Callisto with 0.205º, it is doubted that partial eclipses can occur, because each of the moons’ orbits are so perfectly aligned with Jupiter’s equator; therefore, no partial eclipses. Aside from the types of Jovian eclipses that occur, series of eclipses take place, nevertheless imitating ‘Saros’ here on the earth. Because the moons that do eclipse are rather diminutive compared to Jupiter itself, an observer on Jupiter would not notice much, so a Jovian observer would consider a Jovian eclipse as a phenomena of theoretical interest, or something unimportant to note. Nevertheless, the Jovian moons’ ‘Saros’ is pure academic interest as well.

Seeing a Galilean moon eclipse is an enchanting experience you won’t forget. But, certain requirements are needed for you to observe one; it’s hard for Jupiter to produce such key-viewing times, like the one in 1999. “Jupiter and Saturn returned to the sky in autumn of that year; Jupiter was at its best to view in a long time. Jupiter and its moons were easily observed with a small telescope, and two of three phenomena could easily be seen. Transits and occultations were easy to see, but not so much for eclipses. That’s what makes eclipses so amazing,” Matthew Winter writes from Astronomical Events: Eclipses, Transits, Occultations, and Conjunctions. In order for Jupiter to produce a good eclipse viewing season, it first must be at either eastern or western quadrature. Quadrature is simply a fancy term for the time when a planet forms a right triangle with the earth and Sun. Western Quadrature occurs when the planet is towards the west of earth, and Eastern Quadrature is vice versa. Jupiter forms a twelve degree angle on its end, while the ninety degree angle is on earth’s end. Then, we are able to see the moons eclipse in and out of Jupiter’s shadow cone, rather than at opposition. At opposition, when the earth, Sun, and the planet of note (Jupiter) are all aligned in a straight line, Jupiter’s shadow cone is behind the planet, making eclipses invisible from earth. Precise timings are location is everything in viewing a Jovian eclipse. “Because its shadow cast is very magnificent, when a Galilean moon passes behind it, it disappears completely from view, but has not been occulted. As well as that, because the shadow cast is so steep, the Galilean moons may be viewed entering and exiting the shadow on the same side of the planet!,” from Astronomical Events: Eclipses, Transits, Occultations, and Conjunctions.

Jupiter’s shadow cone is brought into our view at quadrature, it’s not at opposition, which is when Jupiter would make the earth, Sun, and Jupiter in a straight line.
August 1, 2011 brings us to Jupiter’s Western Qudarature, which is a key time to view these events. Around west quadrature, Jupiter rises beautifully in the east around midnight and shines high up at dawn. But mind you, Jupiter takes over eight years to orbit, so returning to Eastern Quadrature will take a few years, so patience is a good aspect in waiting for the return of the Jovian eclipses.  Returning to 1999, Capitol Skies (the newsletter of the Madison Astronomical Society) tells us this about the Jovian eclipses during that epic season. “Jupiter provides a virtual smorgasbord of events to watch. Of the three events, eclipses are by far the most scientifically interesting, because the timing of the precise disappearances and reappearances of the moons can be used to calculate orbital elements of the moons. For this reason, precise timings of the Galilean moon eclipses are sought by the Association of Lunar and Planetary Observers (ALPO).” You can visit a myriad of online resources to locate the times of Jovian eclipses, for what more is there to miss? A moon may be eclipsing now!

Here is a basic explanatory site of Jupiter’s phenomena:

Galilean moons simulator from the Transits Page (click ‘now’ for most current events):

[To download the Word Document of this story, come to this page where it can be downloaded.] 
 
http://astronomicaleventscalendar.blogspot.com/2011/08/understanding-jovian-eclipses.html 

Tuesday, January 17, 2012

Jovian Dual-Shadow Transit for January 18, 2012

In perfect resonance, this January, Ganymede and Europa will dual-shadow transit three times, each a perfect interval apart: one week. Last Wednesday night (approx. 1:30 am EST), the moons will transit, and again, on the 18, the will again; finishing up a week from this transit (the 25). Hopefully, viewing conditions will be perfect tonight, as Wednesday, January 18, 2012's transit will be the longest, in totality, 1:48 hours long, for dual transit, and 1:45 hours long for dual-shadow transit. This is much more "like" a dual-transit, as last's weeks was dull; although no dual-shadow transits are dull, mind you!

According to Simultaneous Transits of Galilean satellites and their shadows across Jupiter during 2012, a paper that lists each of dual-transit phenomena in full (can be accessed here), everything starts at 8:57 UT (3:57 am EST) and ends 10:45 UT (5:45 EST). Although the end of the event might be lost in the morning sunrise, nevertheless the beginning is worth seeing.


Note: If something on the picture reads "Shadow Ingress (or Egress)," and no shadow is seen, this is particularly because of Jupiter's position at this time. The shadows will not be visible until Jupiter moves into another position. 

-all pictures below are credit The Transit's Page, Galilean Moons Simulator; text entered by myself-

2012-Jan-25 09:26 Conjunction of Europa and Ganymede [46.8" E; 6.2" S]



TOTAL EVENTS FOR JANUARY 18, 2012


2012-Jan-18 00:23 Western Elongation of Callisto, 537.8"
2012-Jan-18 05:53 Transit of Great Red Spot
2012-Jan-18 08:36 Transit Ingress of Ganymede
2012-Jan-18 08:38 Shadow Transit Ingress of Ganymede
2012-Jan-18 08:57 Transit Ingress of Europa (Double Transit Begin)
2012-Jan-18 08:58 Shadow Transit Ingress of Europa (Double Shadow Transit Begin)
2012-Jan-18 09:23 Occultation Disappearance of Io
2012-Jan-18 09:43 Inferior conjunction of Ganymede
2012-Jan-18 10:14 Inferior conjunction of Europa
2012-Jan-18 10:43 Shadow Transit Egress of Ganymede (Double Shadow Transit End)
2012-Jan-18 10:45 Transit Egress of Ganymede (Double Transit End)
2012-Jan-18 11:26 Shadow Transit Egress of Europa
2012-Jan-18 11:27 Transit Egress of Europa
2012-Jan-18 11:33 Eclipse Reappearance of Io
2012-Jan-18 12:12 Conjunction of Europa and Ganymede [28.1" W; 5.8" S]
2012-Jan-18 15:49 Transit of Great Red Spot
2012-Jan-18 21:04 Eastern Elongation of Io, 120.6"

Tuesday, January 10, 2012

Jovian Dual-Shadow Transit of January 11, 2012

2012. It is a new year, and what better other way is it to start it off with another dual-shadow transit of Ganymede and Europa!? Although 2012 has less dual-transits than 2011 had, hopefully this year will exceed your expectation on astronomy and Jovian-dual transits. We start the year with a dual-shadow transit of Europa and Ganymede on January 11, 2012 at 4:41 UT. Io will not come into the picture again until March 23; Europa and Ganymede will dual-shadow transit three times in January (the 11, 18 & 25). Callisto does not take any part this year, as it did on January 25, 2011.

According to Simultaneous Transits of Galilean satellites and their shadows across Jupiter during 2012, a paper that lists each of dual-transit phenomena in full (can be accessed here), the January 11 dual-shadow transit is one of the shortest transits of the year, with Europa and Ganymede themselves transiting for 00:23 minutes; both shadows of these moons transit for 00:20 minutes, though. This occurs over the time frame of 06:24 to 06:47 UT for dual-transit, and 06:25 to 06:25 UT for dual-shadow transit. If the skies are clear on the Eastern Seaboard, this event will take place at 1:24 am EST and end on 1:47 am EST. The last two transits (October 24 and 31) were not visible; at last there is one that is, needless to consider others that are coming!

Note: If something on the picture reads "Shadow Ingress (or Egress)," and no shadow is seen, this is particularly because of Jupiter's position at this time. The shadows will not be visible until Jupiter moves into another position. 

-all pictures below are credit The Transit's Page, Galilean Moons Simulator; text entered by myself-

January 10, 2012 at 21:24 UT. You can see that Ganymede and Europa are ready to transit 1/11 at approx. 4:30 UT!

Here Comes Io! Although the above pictures are cropped, Io is in them to the right of Jupiter. Now, it has come in full view as it ascends into occultation by Jupiter itself. Ganymede and Io conjunct right before this occurs, as you can see. 

2012-Jan-11 16:54 Conjunction of Europa and Ganymede [124.5" W; 6.4" S]
You may notice that Europa and Ganymede conjunct twice today (at 16:54 and 19:33). This is becasue of their orbits. They are, in the above picture, practically at the end of their 'orbit,' and will reverse to come behind Jupiter. Doing this, they conjunct again.

TOTAL EVENTS FOR JANUARY 11, 2012

2012-Jan-11 04:39 Transit Ingress of Ganymede
2012-Jan-11 04:41 Shadow Transit Ingress of Ganymede
2012-Jan-11 05:05 Transit of Great Red Spot
2012-Jan-11 05:45 Inferior conjunction of Ganymede
2012-Jan-11 06:24 Transit Ingress of Europa (Double Transit Begin)
2012-Jan-11 06:25 Shadow Transit Ingress of Europa (Double Shadow Transit Begin)
2012-Jan-11 06:45 Shadow Transit Egress of Ganymede (Double Shadow Transit End)
2012-Jan-11 06:47 Transit Egress of Ganymede (Double Transit End)
2012-Jan-11 07:29 Conjunction of Io and Ganymede [19.9" W; 22.2" S]
2012-Jan-11 07:29 Occultation Disappearance of Io
2012-Jan-11 07:40 Inferior conjunction of Europa
2012-Jan-11 08:52 Shadow Transit Egress of Europa
2012-Jan-11 08:53 Transit Egress of Europa
2012-Jan-11 09:39 Eclipse Reappearance of Io
2012-Jan-11 15:00 Transit of Great Red Spot
2012-Jan-11 16:54 Conjunction of Europa and Ganymede [124.5" W; 6.4" S]
2012-Jan-11 19:08 Eastern Elongation of Io, 123.4"
2012-Jan-11 19:33 Conjunction of Europa and Ganymede [151.7" W; 6.9" S]

Saturday, January 7, 2012

2012 Calculations of Dual-Transits are Finally Here!

Thanks to the Transits Page, the 2012 results are finally here! "During 2012 Earth experiences 18 dual satellite and 17 dual shadow transits of Galilean satellites of Jupiter," opens the document. (For comparison, 2011 has 18 dual-satellite but 20 dual shadow.)

http://transit.savage-garden.org/en/horizons/gsst2012.pdf

Longest Dual Transit = 2012 Jul 28 = 02h 02m (Io and Europa)
Shortest Dual Transit = 2012 Jul 10 = 00h 00m (Io and Europa)

Longest Dual Shadow Transit = 2012 Jul 28 = 02h 01m (Io and Ganymede)
Shortest Dual Shadow Transit = 2012 Aug 18 = 00h 08m (Io and Europa)
_____________________________________

Dual Transits

Begin           End               Duration           Satellites

Jan-11 06:24 Jan-11 06:47 00:23 Europa Ganymede
Jan-18 08:57 Jan-18 10:45 01:48 Europa Ganymede
Jan-25 12:38 Jan-25 14:03 01:25 Europa Ganymede
Mar-23 00:30 Mar-23 01:08 00:38 Io Ganymede
Mar-30 03:24 Mar-30 04:43 01:19 Io Ganymede
Jul-10 19:54 Jul-10 19:54 00:00 Io Europa
Jul-14 08:54 Jul-14 09:19 00:25 Io Europa
Jul-17 21:53 Jul-17 22:42 00:49 Io Europa
Jul-21 10:53 Jul-21 12:06 01:13 Io Europa
Jul-24 23:52 Jul-25 01:30 01:38 Io Europa
Jul-28 12:51 Jul-28 14:53 02:02 Io Europa
Jul-30 07:26 Jul-30 09:21 01:55 Io Ganymede
Aug-01 01:52 Aug-01 04:00 02:08 Io Europa
Aug-04 15:16 Aug-04 16:59 01:43 Io Europa
Aug-08 04:37 Aug-08 05:57 01:20 Io Europa
Aug-11 18:00 Aug-11 18:56 00:56 Io Europa
Aug-15 07:21 Aug-15 07:54 00:33 Io Europa
Aug-18 20:43 Aug-18 20:52 00:09 Io Europa

Dual Shadow Transits

Begin        End           Duration       Satellites

Jan-11 06:25 Jan-11 06:45 00:20 Europa Ganymede
Jan-18 08:58 Jan-18 10:43 01:45 Europa Ganymede
Jan-25 12:40 Jan-25 14:02 01:22 Europa Ganymede
Mar-23 00:30 Mar-23 01:06 00:36 Io Ganymede
Mar-30 03:27 Mar-30 04:43 01:16 Io Ganymede
Jul-14 08:54 Jul-14 09:18 00:24 Io Europa
Jul-17 21:54 Jul-17 22:41 00:47 Io Europa
Jul-21 10:53 Jul-21 12:06 01:13 Io Europa
Jul-24 23:52 Jul-25 01:29 01:37 Io Europa
Jul-28 12:51 Jul-28 14:52 02:01 Io Europa
Jul-30 07:29 Jul-30 09:19 01:50 Io Ganymede
Aug-01 01:53 Aug-01 03:59 02:06 Io Europa
Aug-04 15:16 Aug-04 16:58 01:42 Io Europa
Aug-08 04:38 Aug-08 05:57 01:19 Io Europa
Aug-11 18:01 Aug-11 18:55 00:54 Io Europa
Aug-15 07:22 Aug-15 07:53 00:31 Io Europa
Aug-18 20:43 Aug-18 20:51 00:08 Io Europa

Wednesday, November 2, 2011

Results of the October 31, 2011 Jovian Dual Transit

An other amazing spectacle in solar-system astronomy! We must thank again the moons for such a wonderful show - as Io and Ganymede transited this last October 31, 2011. We here in America could not view this event as proficiently as we could have hoped to, but scattered simulations were found all over the web, reminding us of what did occur. Although I could find no pictures of this last transit, (it was very fortunate that I did the last!) here are some computer simulations from all over the web for us to see what did happen. 

"After having such a prolific season of simultaneous Jovian dual-transits last May-June, it will be hard to accept the fact that we have only two more this 2011 season: October 24, 2011 and October 31, 2011. Each transits are an exact week apart (although times differ) and both are dual-shadow transits. Io and Ganymede both partake in each event, as their orbits must be aligned perfectly just for this week." Read more at the link above. (Basic insight of what happened).

31 October 18.23 UT

Here's a simulation from WinJUPOS of what it will look like at 18:15


Below is a picture computed (simulated) by Celestia software. You can see Ganymede and Io as the light blobs, and their shadows cast on the planet. If you would to see the picture clearer, you may click on it for higher resolution. 


Although these are not the most high quality images available, they do beautifully illustrate the beauty of this transit. So, just to say - I will hopefully be receiving the 2012 Galilean moons calendar soon - so until next year....

Saturday, October 29, 2011

Jovian-Dual Shadow Transit for October 31, 2011

Remarkable was the dual-shadow transit on October 24. But, there is yet another and unfortunately the final dual-shadow transit of Jupiter in 2011. October 31 will bring us one more "astronomical morsel" and this one will be presumably about the same as the last: Io will transit just beneath the waistline of Jupiter, and Ganymede at the exact bottom of the king of the planets. Both of the shadows will be cast on the planet for only sixteen minutes, from 18:10 to 18:26 UT. This will be during the day for Washington DC, at approximately 1:10 to 1:26 EDT. Although this is rather sad, the eastern world will be able to witness the last Jovian dual-transit for the great year of 2011. A comprehensive photo shoot (courtesy of The Transits Page) is shown at the end of this article. Below is a picture of the Jovian moons at 00:00 UT on October 31, 2011, or at 8:00 October 30, for us here in EDT.

Image Credit: Transits Page; Text entered by AstronomicalEventsCalendar

Callisto beautifully rests on top of the planet, as it's orbit appears to be above the planet, we must remember that these orbits are three dimensional - and that since Jupiter is titled towards us, it looks like Callisto orbits above. Sense Perception! Concerning the transit, you can see Io and Ganymede - Ganymede will swoop down and catch up to Io (they are not actually that far apart in the two-dimension scale, becasue of their orbits, but they appear to be far apart). The dual-transit itself will start at 17:46 UT and end at 18:22 UT, lasting only 36 minutes. If you can remember, this is very shorter than the October 24 transit.The next picture below concerns itself right before the transit - at 16:00 UT. Ganymede and Io are now very noticeable together.

Image Credit: The Transits Page; Text entered by AstronomicalEventsCalendar

If you're wondering what a Jovian dual-sahdow transit is? Look no further - Here, we can clarify the terms of dual-shadow transit, and dual-transit, becasue both can happen at the same time - the October 24 and 31 transits are great examples of these (among others). A dual-shadow transit occurs when two shadows of moons travel across the surface of Jupiter together (and yes this can also happen on any other planet with two or more moons, etc.), and then, when the two moons travel together, it is called a dual-transit. (The difference is just either the shadow or moon), but both have to cross Jupiter (or any other planet, etc.) at the same time. You can read more about Jovian transits in our last transit: October 24.

-all pictures below are credit The Transit's Page, Galilean Moons Simulator; text entered by myself-



Another object to note is the conjunction of Io and Ganymede again, but the next day:
2011-Nov-01 05:19 Conjunction of Io and Ganymede [144.0" W; 21.7" S].


TOTAL EVENTS FOR OCTOBER 31, 2011
2011-Oct-31 15:12 Conjunction of Io and Ganymede [44.7" E; 13.1" S]

2011-Oct-31 16:13 Transit Ingress of Io (All satellites no more visible to the east of Jupiter)
2011-Oct-31 16:18 Shadow Transit Ingress of Io
2011-Oct-31 17:18 Inferior conjunction of Io
(2011-Oct-31 17:45 Conjunction of Callisto and Europa [204.4" E; 38.1" S])*
2011-Oct-31 17:46 Transit Ingress of Ganymede (Double Transit Begin)
2011-Oct-31 18:10 Shadow Transit Ingress of Ganymede (Double Shadow Transit Begin)
2011-Oct-31 18:22 Transit Egress of Io (Double Transit End)
2011-Oct-31 18:26 Shadow Transit Egress of Io (Double Shadow Transit End)
2011-Oct-31 18:30 Inferior conjunction of Ganymede
2011-Oct-31 19:09 Transit Egress of Ganymede
2011-Oct-31 19:24 Shadow Transit Egress of Ganymede

*Object of Note!
(with thanks to the Galilean Moons Simulator)

Tuesday, October 25, 2011

Results of the October 24, 2011 Jovian Dual Transit

The dual-shadow transit on October 24, this past Monday was a true spectacle! Although we here in America could not view such a wonderful event, I have been able to find a few pictures scattered across the internet of this spectacular event. About the transits: "After having such a prolific season of simultaneous Jovian dual-transits last May-June, it will be hard to accept the fact that we have only two more this 2011 season: October 24, 2011 and October 31, 2011. Each transits are an exact week apart (although times differ) and both are dual-shadow transits. Io and Ganymede both partake in each event, as their orbits must be aligned perfectly just for this week." Read more at the link above.

This picture was taken from 'Cloudy Night Telescope Reviews' under username 'claytonbigwood'

Below is a picture computed (simulated) by Celestia software. You can see Ganymede and Io as the light blobs, and their shadows cast on the planet. If you would to see the picture clearer, you may click on it for higher resolution.


Although these are not the most high quality images available, they do beautifully illustrate the beauty of this transit. Remember that October 31 brings us another galactic delicacy! Another dual-shadow transit awaits us...

Saturday, October 22, 2011

December 27, 2011 Dual-Shadow Transit

According to the "Robert Ferguson Observatory," they state in their 2011 Observing highlights, that there will be a dual-shadow transit of Europa and Ganymede on December 27, 2011. Although I do recommend their observing highlights to those who would like to know, their event is incorrect. They have:

  • Tuesday, 12/27/2011 - Dbl Sh Tr Jup - Time: 18:00
    • Double shadow transit of Jupiter:
      Transit of Europa is already in progress at sunset.
      06:00p Nautical twilight ends
      06:05p Ganymede's shadow begins transit
      06:32p Astro twilight ends
      07:44p Io is occulted by Jupiter
      07:51p Europa's shadow begins transit
      07:52p Europa transit ends
      07:55p Ganymede's shadow transit ends
      10:15p Europa's shadow transit ends
      11:07p Io reappears from eclipse

Although I do not wish to refute this prediction, after checking the Galilean moons simulator, they're prediction is wrong. Ganymede does transit and Io does eclipse, but Europa is just too far away from Ganymede for dual-shadow transit. Without making any advanced Judgments, this may occur, but maybe if viewed from a different angle on the earth.

Computer Simulation of Galilean moons provided by the Galilean Moons Simulator, Text Inserted by AstronomicalEventsCalendar

Wednesday, October 12, 2011

Jovian Dual-Shadow Transit of October 24, 2011

After having such a prolific season of simultaneous Jovian dual-transits last May-June, it will be hard to accept the fact that we have only two more this 2011 season: October 24, 2011 and October 31, 2011. Each transits are an exact week apart (although times differ) and both are dual-shadow transits. Io and Ganymede both partake in each event, as their orbits must be aligned perfectly just for this week. According to Simultaneous Transits of Galilean satellites and their shadows across Jupiter during 2011, a paper that lists each of dual-transit phenomena in full (can be found here), the October 24 dual-transit is the longest of the two (the other being October 31, respectively) with both moons transiting over 1 hour 18 minutes, with both shadows on the planet over the span of 58 minutes. A comprehensive photo shoot (courtesy of The Transits Page) is shown at the end of this article.

Image Credit: Transits Page; Text entered by AstronomicalEventsCalendar

Looking at the above image, we see the Galilean moons on October 24, 2011 at 00:00 UT (times forth are Universal Time, or UT). The transit begins 14:22 UT and ends comprehensively at 15:20 UT - a rather long dual-transit at 1 hour and 28 minutes, although the longest was on January 10, 2011 (2 hrs & 15 min). The next image shows the Jovian satellites at 14:00 UT, on the same date. Note how close Io and Ganymede are, and the shifting of Callisto and Europa.

Image Credit: The Transits Page; Text entered by AstronomicalEventsCalendar

In the above image, you can see Io and Ganymede about to enter transit. Callisto has shifted further away from Jupiter as it completes its orbit, and Europa is shifting down, as its orbit is completed. During transits with Ganymede, because of Ganymede's orbital eccentricy, it orbits near the south pole of Jupiter, making transits involving it shorter than transits with Europa. Europa and Io orbit very closely around the belt line of Jupiter, making dual-transits more facile; Callisto only dual-transited once this year, on January 10 (which was the longest, partially becasue Callisto is the farthest moon, and orbits slower than Europa, who shared the transit. Other than that, only Io transits the rest of 2011, with either Ganymede or Europa, see for yourself here.)

Before the transit begins, at 04:19 UT, Io and Ganymede will conjunct, as the picture below (first) shows us. Celestial Coordinates: [145.1" E; 20.6" S]. On the timing of the transit, Ganymede's shadow will ingress first at 14:06 UT (note before the actual dual-transit begins), and then Io's will at 14:22, signifying the start of the dual-transit. From there, Io will start its journey across Jupiter's luminous disk at 14:29 UT, and Ganymede at 14:34, starting the dual-transit of the moons.

Here, we can clarify the terms of dual-shadow transit, and dual-transit, becasue both can happen at the same time - the October 24 and 31 transits are great examples of these (among others). A dual-shadow transit occurs when two shadows of moons travel across the surface of Jupiter together (and yes this can also happen on any other planet with two or more moons, etc.), and then, when the two moons travel together, it is called a dual-transit. (The difference is just either the shadow or moon), but both have to cross Jupiter (or any other planet, etc.) at the same time.

You can see most of the events of this transit below, computer simulated, becasue 14:22 UT is 10:22 EDT; we here in America will not be able to view this transit (neither the 31). You can convert times here. {This is a rather sad fact for us here in America, but for those in East Asia, the Pacific, and some of the Middle East will enjoy seeing this treat. Jupiter here in America is high during night - and at Opposition, and it's very sad that we won't be able to see it!}

-all pictures below are credit The Transit's Page, Galilean Moons Simulator; text entered by myself-










TOTAL EVENTS FOR OCTOBER 24, 2011

2011-Oct-24 00:16 Conjunction of Europa and Ganymede [194.4" E; 27.3" S]
2011-Oct-24 04:19 Conjunction of Io and Ganymede [145.1" E; 20.6" S]
2011-Oct-24 04:48 Transit of Great Red Spot
2011-Oct-24 05:00 Eastern Elongation of Io, 145.9"
2011-Oct-24 08:27 Eastern Elongation of Europa, 235.1"
2011-Oct-24 14:06 Shadow Transit Ingress of Ganymede
2011-Oct-24 14:22 Shadow Transit Ingress of Io (Double Shadow Transit Begin)
2011-Oct-24 14:29 Transit Ingress of Io
2011-Oct-24 14:34 Transit Ingress of Ganymede (Double Transit Begin)
2011-Oct-24 14:44 Transit of Great Red Spot
2011-Oct-24 15:16 Inferior conjunction of Ganymede
2011-Oct-24 15:20 Shadow Transit Egress of Ganymede (Double Shadow Transit End)
2011-Oct-24 15:34 Inferior conjunction of Io
2011-Oct-24 15:52 Transit Egress of Ganymede (Double Transit End)
2011-Oct-24 16:09 Conjunction of Io and Ganymede [12.5" W; 13.1" S]
2011-Oct-24 16:30 Shadow Transit Egress of Io
2011-Oct-24 16:38 Transit Egress of Io

(With thanks to Galilean moon Simulator).

Monday, October 10, 2011

Last Two Jovian Dual-Transits for the 2011 Season

Although it is rather sad, the last two Jovian dual-transits will take place respectively on October 24 and 31, 2011; always a sempiternal treat! Apparently, the Jovian moons are falling back to imperfect resonance (to cause them not to be aligned perfectly), but the orbits are never too imperfect; more than likely, their orbital Saros has ended. It is a misconception to think that only earth's moon has a Saros, but indeed other moons do as well. For eclipsing (or transiting, respectively!) all moons need a Saros pattern, and even though one hasn't been established (that I am aware of), it still follows this Saros.

Figure 1 - The Orbital Resonance of the Jovian moons.

A Jovian dual-transit is a rare and exciting phenomena that occurs when two (or more) of the Jovian moons pass in front of Jupiter, passing together and usually casting shadows. Below is such an example, and below that is a picture of a Jovian triple-transit; quite an event.

May 7, 2011 dual transit provided by the transits page.

March 28, 2004 triple Jovian transit. The fourth black dot is actually a moon itself, casting a shadow.

As we begin to wait for the moons to dual-transit one last time in 2011, let us make known the occurrence of such events. In the Dual-Transits Ephemeris provided by the transits-page, in 2011, eighteen dual transits occur, but twenty dual-shadow-transits occur. This is important to note: the difference between the dual-shadow transit and the plain dual-transit.

Jovian dual-transit - the transit of two or more Jovian moons across the face of Jupiter, usually very long due to the fact of their shadows

Jovian dual-shadow transit - the transit of two or more Jovian moons across the face of Jupiter, with shadows, so the length would be shorter

According to these definitions, if two moons transit, with two shadows transiting as well as moons (Jovian dual-shadow transit) four spots may appear on the planet (Jupiter), though most of the time it's just the shadows that occur. You can read more at the link provided above. More information will be provided in the coming days - ON THIS SITE. Thank you!

Credit: NASA